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Peta–electron volt gamma-ray emission from the Crab Nebula

Peta–electron volt gamma-ray emission from the Crab Nebula
Written by Emma Kent

The Crab Nebula is a bright source of gamma rays powered by the Crab Pulsar’s rotational energy through the formation and termination of a relativistic electron-positron wind. We report the detection of gamma rays from this source with energies from 5 x 10–4 to 1.1 peta–electron volts with a spectrum showing gradual steepening over three energy decades. The ultrahigh-energy photons imply the presence of a peta–electron volt electron accelerator (a pevatron) in the nebula, with an acceleration rate exceeding 15% of the theoretical limit. We constrain the pevatron’s size between 0.025 and 0.1 parsecs and the magnetic field to 110 microgauss. The production rate of peta–electron volt electrons, 2.5 x 1036 ergs per second, constitutes 0.5% of the pulsar spin-down luminosity, although we cannot exclude a contribution of peta–electron volt protons to the production of the highest-energy gamma rays.

Read original article here: Peta–electron volt gamma-ray emission from the Crab Nebula

Read original article here: Peta–electron volt gamma-ray emission from the Crab Nebula



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